H-Alpha

Use a DSLR Ha Filter for Astrophotography

After almost a decade of taking pictures of space with a DSLR camera, I have come to the realization that a DSLR Ha filter is the quite possibly the most important astrophotography filter in your kit. Traditional light pollution filters designed to help you photograph deep sky objects in broadband (true-color) are useful, but a hydrogen-alpha filter makes the single greatest impact on your astrophotography overall.

Beginners often ask me which narrowband filter (line filter) I recommend to buy first, and it’s always an Ha (or “Hα”) filter. H-alpha is a specific deep-red visible spectral line with a wavelength of 656nm. Many nebulae in the night sky (and even some galaxies) emit a strong signal of light in this wavelength and a hydrogen alpha filter helps to isolate and record this signal with your DSLR camera.

In this post, I’ll explain why a clip-in DSLR h-alpha filter is not only the most powerful filter in your kit, but the one you’ll probably use the most. The DSLR Ha filter I use and recommend is the Astronomik 12nm Ha filter (Canon EOS). There are several versions of this clip-in DSLR filter available, including models for Canon full frame bodies like the popular Canon EOS 6D and 6D Mark II.

All of these images were captured with a Canon DSLR and an Astronomik 12nm Ha filter.

Not a fan of black and white images? No problem, use the data you collect in Ha as a powerful luminance layer to your color images. As with other narrowband filters, such as O III and S II, capturing data from a precise bandpass offers many creative opportunities to improve your existing images.

I’ve previously covered narrowband filters that collect multiple wavelengths (dual bandpass, quad bandpass etc.). This time, I’m focusing on the most important emission line of them all, hydrogen alpha.

The Effectiveness of a DSLR Ha Filter

Before I share my 7 reasons why I think everyone who shoots with a DSLR camera should have an h-alpha filter, I want to highlight what I believe is the most important feature of all. You can use a clip-in hydrogen alpha filter with a camera lens, and images collected in h-alpha through a short focal length are absolutely breathtaking.

I’ve reviewed many astrophotography filters in the past, including broadband (or “broad spectrum”) filters that help to achieve a natural looking image from a light polluted sky. With so many incredible types of filters out there, how can one filter possibly be of any more useful than the rest?

Here are 7 compelling reasons:

You can capture images during any moon phase

You can add dynamic details to existing color images

Stars are recorded smaller and sharper

Fast f-ratios (F/2.8) can be used without star bloat

A clip-in Ha filter can be used with a camera lens

You can use an h-alpha filter on a stock DSLR (signal is much weaker)

Single bandpass filters are usually more affordable than a multi-bandpass version

Have you ever seen your backyard sky through an h-alpha filter? It’s a pretty astonishing. You can finally see the hidden structure of the Milky Way behind the veil of light pollution in the city. Here is a photo of the constellation Cygnus from my Bortle Scale Class 8 backyard using a 17mm camera lens.

Although the 48mm (2″) filter format can be utilized in more imaging configurations (such as a dedicated astronomy camera) a DSLR clip-in filter fits underneath your camera lens.

Taking wide field astrophotography images using a camera lens in place of a telescope is one of the most rewarding experiences in this hobby. For example, I captured this image of the North America Nebula under a nearly full moon using the Rokinon 135mm F/2.0 ED UMC lens.

The North America Nebula (& Pelican Nebula) captured using an h-alpha filter and 135mm camera lens.

You can use a clip-in DSLR filter with a telescope as well, making it a practical solution for amateur astrophotographers looking to collect narrowband data. The key to the image acquisition stage, is to expose the images long enough so that the histogram shows that the data is separated from “the wall”.

Optical systems with faster f-ratios, whether it’s a telescope or a camera lens, are better suited for narrowband astrophotography with a DSLR. The slower the focal ratio of your lens, the longer the exposure will need to be to adequately expose the image in h-alpha.

For reference, here is a look at a single, unstretched (linear) sub-exposure of the a DSLR image captured in Ha. The data observed in the red channel is the most important, as this is where all of the useful image data lies.

A single 3-minute exposure from a DSLR camera using an H-Alpha filter.

Notice how the entire image has a red cast over it? If you look at the histogram, you’ll see that the majority of the signal (light) has been captured in the red channel. The signal in the blue and green channels is almost non-existent.

Narrowband H-alpha with a DSLR

You may be asking yourself, is it worth it to use an h-alpha filter with a DSLR?After all, the experts in the astrophotography forums will tell you that you can’t use a narrowband filter with a color camera and if you do, you’re crazy.

Perhaps I am crazy, but I have personally enjoyed shooting narrowband images with a color camera for many years and I’ve been thrilled with the results (…maybe my standards are too low?)

The truth is, you can capture and stack narrowband images taken with your one-shot-color DSLR, RGB bayer filter and all, in DeepSkyStacker. Once the images have been registered and stacked using calibration frames, you should end up with an intermediate file that looks a little something like this:

The stacked result of 51 exposures using a DSLR camera and h-alpha filter.

From here, you can bring the stacked TIF file into Adobe Photoshop to extract the red channel and process in the monochrome image.

Use a Clip-In Filter with a Camera Lens

One of the most understated benefits of a clip-in Ha filter is the ability to capture h-alpha images with a camera lens attached. This opens the door to impressive, wide field projects revealing the hidden H II gases in the night sky. Combining the Astronomik 12nm Ha filter with a 135mm lens is an incredibly effective combination.

A clip-in filter is a convenient solution when using a camera lens for astrophotography.

Some telescopes, like the William Optics RedCat 51, include an internal threaded slot for a 48mm filter in the imaging train. However, the only possible spot for an h-alpha filter with a camera lens attached to your DSLR is inside the camera body.

Narrowband filters designed to thread externally to the large lens objective are not common, are a filter of that size (77mm) would be very costly. The Astronomik clip-in filters snap into the body of the DSLR securely, and most lenses will fit on top (be sure to check the compatibility of the lens you intend to use).

I’ve used the Astronomik 12nm clip-in Ha filter with several cameras lenses including the “nifty fifty” (Canon EF 50mm F/1.8), and the ultra wide-angle Rokinon 14mm F/2.8. Here is a look at Barnard’s Loop captured using the clip-in Ha filter in my Canon EOS Rebel T3i.

How To Process the Images

Capturing images using a clip-in hydrogen alpha filter with your DLSR is a lot of fun. No matter how light polluted your skies are, and how bright the moon is, you should see the distinct features of your deep sky object that are emitting light at the 656nm bandpass. Since DSLR cameras collect light through a Bayer filter, the signal is divided up into RGB channels that would normally build a full color image.

However, the h-alpha emission line is very specific, and will only record useful data in the red channel of your images (the other channels will be almost 100% noise). Knowing this, we need to extract the data from the red channel only, and process that channel as a monochrome image of its own.

Stack, Register and Calibrate the Image

The first step is to stack, register, and calibrate your raw images the way you normally would with a color images taken with your DSLR camera. This includes using darks, flats and bias frames to help produce a calibrated image with a healthy signal to noise ratio.

The sub exposures will look extremely red as shown in the example above, and so will the intermediate file that DeepSkyStacker spits out.

Extract the Red Channel in Adobe Photoshop

After opening your stacked TIF file in Adobe Photoshop, open up the Channels Tab (If you do not see this tab, click on Window > Channels from the main menu), and have a look at the data. You should see that almost all of the pixel information resides in the red channel.

Process the Grayscale Image

The image pasted should default to grayscale mode, with only one channel (gray) in the Channels Tab. You can process this image the same way you would a color image, including adjusting the levels, curves, and even using dedicated astronomy actions.

From here, you can either save and share the image as a black and white hydrogen-alpha photo (which are beautiful, by the way), or you can apply this image to an existing color image to give it a dramatic punch. (See my HaRGB Tutorial).

The Difference H-Alpha Makes

Some of the most incredible DSLR deep-sky images ever produced, were created using narrowband filters to isolate specific emission lines in the visible spectrum. You can use the same signal isolating techniques to enhance your existing RGB data.

A narrowband filter lets the h-alpha light of emission nebulae pass through to the camera sensor, and blocks almost all of the other wavelengths of light in the visible spectrum.

To be more specific, the Astronomik 12nm Ha filter allows 97%+ transmission of the H-Alpha line, and blocks nearly the entire remainder of the visible spectrum. This includes blocking unwanted wavelegnths in IR (infrared).

For objects like the Bubble Nebula (shown below), you an collect impactful signal that can be applied to your broadband images.

What does this mean?

It means that city light pollution and moonlight are largely ignored. This opens up the doors to imaging during the full moon, and from a city backyard. You no longer have to wait for the full moon/nearly full moon phases to pass to capture deep sky astrophotography images.

Emission Nebulae and Hydrogen-Alpha

Emission nebulae are clouds of glowing H II gas, and they emit light at a very specific wavelength. This information is beneficial to astrophotographers, as we are able to isolate this wavelength for photography. The light from an emission nebula is created when the atoms in the gas are ionized by the formation of hot young stars.

The dominant wavelength in a hydrogen nebula is the deep red portion of the spectrum known as the hydrogen-alpha line (656nm to be exact).

The Visible Spectrum – Wavelengths in Nanometers

Why this is important for DSLR astrophotography

By using a Ha filter in your DSLR, it is possible to increase the contrast between objects in the h-alpha emission line and the skyglow background. The filter completely suppresses the emission lines of artificial lighting such as mercury (Hg) and sodium (Na).

The particulars of the Astronomik ha filter can be understood in the transmission graph below. The chart shows that the Astronomik filter allows 97% transmission of the h-alpha wavelength

Images captured using a narrowband Ha filter have some pleasing characteristics.

At the top of the list is reduced star size. This further emphasizes the detail and contrast of a deep-sky image by allowing it to stand out from the surrounding sea of stars.

Filtering out skyglow and light pollution means that longer exposure times of 5 minutes and beyond from the city are possible from the city. You will likely capture more detail in your emission nebula targets than ever before.

Challenges and Best Practices in the Field

Earlier in the post, I mentioned that you’ll want to shoot exposures that capture enough signal to produce a quality image. Specifically, you’ll need to make sure that the red channel data is not being clipped in shadows portion (left-hand side) of the histogram.

Slower optical systems will demand longer exposures to reach this value, and that puts added importance on tracking accuracy and the need for autoguiding. If your telescope is in the F/6-F/7 range or slower, expect to collect images that are at least 3-minutes or more to create a useful sub exposure.

This is one of the many reasons I recommend using a DSLR Ha filter with a camera lens like the Rokinon 135mm F/2.0. A fast aperture lens will collect more light in a single shot, and suddenly only a 2-minute exposure is enough to collect a healthy SNR.

Framing and Focusing Targets

The light blocking qualities of narrowband filters means that you will no longer see faint stars through the viewfinder of your DSLR, or when using the live-view function. This can make finding targets and focusing your camera lens or telescope difficult.

In the image below, you’ll see an example of what a single test exposure of about 30-seconds may look like at ISO 1600. There is really only one bright star, and a very faint indication of nebulosity in a 30-second image.

To frame up my image of the North America Nebula, I used a bright star (Deneb) as a reference.

I find that the most practical solution to this challenge is to find the closest, bright star to your intended deep sky object as a point of reference. Even using a 7nm Ha filter (which is stronger and more targeted than the 12nm version), the brightest stars in the night sky will still show up in live-view.

The camera settings must be set to expose as bright an image as possible, which is typical of any framing and focusing routine with a DSLR. Use ISO 6400 or greater, with the maximum aperture of the camera lens. Make sure the camera is set to bulb exposure mode, so let it is letting as much light as possible.

Once you have located a bright star (you can use the Moon, too), take your time focusing the star using the 10X zoom in live-view. If you are using a camera lens, you may want to use tape to secure the focus adjustment ring to avoid knocking it out of position in the next step.

Use a planetarium mobile app or a physical star map to locate the rough position of your target. If you’re lucky, there will be a bright star near your nebula to use as a reference like my example of NGC 7000 above. If not, you may need to take as many as 10+ test shots before you are happy with the framing of your target.

A 30-second exposure at ISO 6400 should be more than enough time to indicate where the areas of hydrogen gas are concentrated.

Choices – 12nm or 6nm versions

The 6nm version of the Astronomik Ha filter has an extremely narrow emission-line filter. This version targets an even narrower portion of the visible spectrum, blocking nearly the whole remainder of the spectrum. So wouldn’t the 6nm version the obvious choice?

Despite the increase in contrast and more light-blocking power of the 6nm version, there were a few reasons I went with the 12nm. For starters, the 6nm version is more expensive, and that was a big reason why I decided to invest in the 12nm filter.

A major step in my pre-imaging routine includes framing my deep-sky target to include as much of the object and surrounding elements as possible. BackyardEOS or Astro Photography Tool can streamline this task with the frame and focus feature.

It’s not the end of the world, but it does take longer to get up and running that it would using a broadband filter that allows more light to reach the sensor. The 6nm would double these impacts, and increase this setup time.

Many backyard astrophotographers would disagree, wishing they had gone with the 6nm instead. I’ve shot images using a 7nm Ha filter (Optolong 7nm Ha), and the results are not drastically different. There is more contrast in the images that used a 6nm filter, but the exposures also need to be longer.

List of Compatible Canon EOS Cameras:

Here is the official camera compatibility list for the Astronomik clip-in Canon EOS Ha filter directly from the High Point Scientific website. I have personally used this Hα filter on a number of Canon camera bodies including full spectrum modified Canon EOS Rebel Xsi and T3i’s, and a stock Canon EOS 7D.

7D

7D Mark II

20D

20Da

30D

40D

50D

60D

60Da

70D

77D

80D

300D (Rebel)

350D (Rebel XT)

400D (Rebel XTi)

450D (Rebel XSi)

500D (Rebel T1i)

600D (Rebel T3i)

700D (Rebel T5i)

750D (Rebel T6i)

760D (Rebel T7i)

1000D (Rebel XS)

1100D (Rebel T3)

1200D

1300D

100D

200D

Lens Compatibility

The Astronomik clip-in hydrogen alpha filter is not compatible with Canon EF-S mount lenses. The EF-S series of Canon lenses were designed to be used solely with Canon APS-C (crop) sensor DSLR’s, and have a smaller image circle.

They fit deeper inside of the camera body, which means that they’ll run into the height of the filter if you try to attach the lens. In the photo below, you can see how the base of the lens mount is protruding too far to be compatible with a clip-in DSLR ha filter.

Stick to full frame lenses on your crop sensor DSLR. The EF-S lens mount wont work with a clip-in filter!

On the other hand, Canon EF series lenses were designed to be used with both full frame camera bodies and crop sensor models. I’d recommend sticking with EF lenses for astrophotography in general, from a quality perspective.

I enjoy Canon’s L-series lenses, which is why several years ago I began purchasing used l-series lenses to cover every possible photography situation. Third party full frame lenses with the EF mount design such as the Rokinon 135mm F/2.0 ED UMC I mentioned earlier are compatible with DSLR clip filters like this.

Stick to full frame lenses such as the Canon EF line up and the many thir party lenses that mount to Canon cameras from Rokinon, Samyang, Sigma etc. One way to tell if your lens is a suitable design for Canon clip-in DSLR filters, is the small red indicator at the base of the lens.

Does my camera need to be modified for astrophotography?

No. The same benefits of an H-alpha filter can be realized with a stock DSLR. However, the amount of red light your camera will be able to record will be reduced.

If you are serious about your astrophotography, it is worth thinking about modifying your camera either yourself or by a professional. Here is a shot of the Eagle nebula using the Astronomik Ha filter and a stock Canon EOS 7D.

Example of using a Ha filter with a stock (unmodified) DSLR camera (Canon EOS 7D).

This is typically what a frame looks like taken using a Ha filter through an unmodified DSLR. This emission nebula could have been captured in greater detail using a modified camera, but the skyglow and wavelength suppression capabilities of the filter are still present.

I am a huge promoter of DSLR astro-mods. If your camera is used for astrophotography exclusively, why not modify your camera yourself? That’s exactly what I did to my Canon EOS 450D (Rebel Xsi) camera in 2014.

I carefully removed the IR cut filter on my Canon Rebel 450D by watching this video from Gary Honis. If you have either a light pollution or h-alpha filter covering your DSLR sensor at all times, you are not required to install any extra replacement filters.

This is known as a full spectrum “naked sensor” mod, and it made a huge impact on my astrophotography images.

The Bottom Line

If you own a DSLR camera that has been modified for astrophotography, a clip-in Ha filter should be on your shopping list. I waited far too long before making this decision.

Combining H-alpha exposures to your existing RGB data can greatly increase the amount of detail and contrast in your nebula images, and even add dramatic details to certain galaxies.

The ability to image during the full moon and surrounding week results in much more time under the stars. No more wasted moonlit clear nights.

If you live in the city, a Ha filter cuts through even the most severe light pollution. My Astronomik 12nm Ha filter cuts through my red-zone (Bortle Class 8) skies to reveal beautiful structures of hydrogen gas in the emission nebulae I photograph.

Narrowband filters allow you to collect impressive deep sky images from a light polluted backyard, and that’s a beautiful thing.

The clip-in versions offered by Astronomik are a perfect fit for several Canon and Sony cameras.

This month, I have been getting a head start on summer Astro targets in Sagittarius such as the Omega Nebula. This means waiting until after midnight for my targets to rise high enough in the Southeast for a clear view.

The Canon Rebel T3i is back in action!

Despite the glow of the full moon and nightly “lows” of 27 degrees Celsius, I have continued to fire away at the night sky with my modified Canon DSLR.

H-Alpha with a DSLR: Crescent Nebula

The Crescent Nebula in H-Alpha

The subject of my most recent outings is NGC 6888 in Cygnus, the Crescent Nebula. With an Astronomik 12nm ha filter installed in my Canon 600D, I have captured over 3 hours worth of data on this striking emission nebula.

My version of NGC 6888 is just starting to show the fainter details of the nebula. A deeper view like this one featured on Astronomy Magazine shows the delicate structure of this deep sky object.

As I mentioned earlier, these were HOT nights. The temperature of the camera sensor was well over 30 Degrees Celsius for most of these images. This is quite a drastic contrast between the chilly images I captured last month using the icy ASI071MC-Cool.

The Crescent Nebula in H-Alpha

Imaging Session 1 – June 10

Canon T3i @ ISO 800
300-second subs

Imaging Session 2 – June 11

Canon T3i @ ISO 1600
300-second subs

The Crescent Nebula is a notoriously difficult deep sky target from light polluted locations. Those shooting with a stock DSLR may be disappointed by the lack of structure captured using modest exposure lengths. Dark skies and hour of data are essential to produce a detailed portrait of NGC 6888.

Image Processing (Video)

The video below has been sped up to show you the basic image processing steps I took in Adobe Photoshop. The image starts out as the RAW stacked file produced by Deep Sky Stacker – and is processed using levels, curves and specific actions from the Astronomy Tools Action Set.

Collecting Color (RGB) Data

This Ha data will later be combined with upcoming true color RGB photos to produce an HaRGB composite in Photoshop. The hydrogen alpha details in the Crescent Nebula should help boost contrast in the final image.

Later, I’ll use the SkyTech CLS-CCD light pollution filter to capture my broadband RGB data with the 600D. This filter does a great job at separating the nebula from the washed out background sky.

To combat the thermal noise in my images, all I can do is limit the ISO sensitivity when shooting, and apply dark frames when stacking in Deep Sky Stacker.

As expected, the RAW images out of the camera were incredibly noisy. Stacking multiple images and subtracting darks certainly helped, but it does not correct the issue completely.

This is precisely why I am so interested in the capabilities of the Altair Astro Hypercam 183C, and how the Sony IM183 sensor will perform.

The Hypercam 183C will take over as my primary imaging camera starting this week

The nebula looks gorgeous in Ha, but what about color? Below is an example of this target using a stock digital camera in full color.

NGC 6888 through a stock Sony A6300

A member of the AstroBackyard Facebook page recently shared his image of the Crescent Nebula using a stock Sony Mirrorless digital camera. This is a great example of what to expect using a stock Sony A6300 for astrophotography.

NGC 6888 using a Sony A6300 mirrorless camera

Zhonghua was able to pull out some impressive detail and color in this faint emission nebula with his stock A6300. This was captured through a Celestron NexStar 6SE telescope on a custom built wedge mount.

The image above shows the Crescent nebula in true color, which I will be adding to my original H-Alpha image for an HaRGB composite. This way, I am able to show the nebula in true color, while benefitting from the additional contrast and detail in the hydrogen alpha wavelength.

The Summer Triangle

The constellation Cygnus, including NGC 6888 is a part of an asterism in the night sky known as the “Summer Triangle“. This triangle of stars consists of Altair, Deneb, and Vega.

By mid-July, these imaging sessions will commence when the night has set in at about 10:30 pm. I enjoy watching the Summer Triangle continue its approach into my backyard viewing window night after night.

The Summer Triangle consists of Altair, Vega, and Deneb

Anything I photograph in this region is arguably the darkest and clearest area of the sky from my backyard. The photo above was shot through heavy light pollution using a wide angle camera lens. Through careful image processing, I am able to restore the details of this dense region of the Milky Way.

Testing the Hypercam 183C

The highly anticipated Hypercam 183C astronomy camera will be arriving this week. Although the CMOS IMX183 sensor is not cooled via TEC-cooling, it benefits from an internal fan and a design that maximizes air flow.

You can expect some color images of the Crescent Nebula using the 183C in the coming weeks. The team over at Ontario Telescope and Accessories have assured me that 183C is on the way!

The 20MP sensor housed in the Hypercam means that the resolution will exceed the current size of my Rebel 600D image frames. Some scaling will be required to match the images up in the image processing stage